莎草 发表于 2025-3-26 22:44:01
http://reply.papertrans.cn/33/3219/321831/321831_31.pngchondromalacia 发表于 2025-3-27 04:17:24
http://reply.papertrans.cn/33/3219/321831/321831_32.png截断 发表于 2025-3-27 05:28:09
http://reply.papertrans.cn/33/3219/321831/321831_33.pngCommon-Migraine 发表于 2025-3-27 10:26:30
Macroscopic perturbations of the IMF by P/Halley as seen by the Giotto magnetometeralley the IMF showed quite a stable “away” polarity. Draping of magnetic field lines is clearly observed along the outbound leg of the trajectory. Inside the magnetic pile-up region the field reverses its polarity several times. A symmetry of oppositely magnetized sheets with respect to the nucleus博识 发表于 2025-3-27 17:00:56
http://reply.papertrans.cn/33/3219/321831/321831_35.pngfidelity 发表于 2025-3-27 20:23:40
http://reply.papertrans.cn/33/3219/321831/321831_36.png泥沼 发表于 2025-3-28 00:20:57
http://reply.papertrans.cn/33/3219/321831/321831_37.pngInvigorate 发表于 2025-3-28 05:22:53
http://reply.papertrans.cn/33/3219/321831/321831_38.png奇怪 发表于 2025-3-28 07:15:01
http://reply.papertrans.cn/33/3219/321831/321831_39.pngenfeeble 发表于 2025-3-28 13:57:49
Plasma flow in the cometosheath of P/Halley during the encounter of Suiseiexcept near the bow shock and that of alpha particle was almost constant (~ 7 cm.) in the cometosheath. Temperature of protons seems to decrease from bow shock to about 2 10. km, and increase thereafter slightly, but that of alpha particle seems to be almost constant. This decrease is likely caused